2024RNAAS...8..218S

Dust polarization observations of starlight at multi-wavelengths helps us to find maximum polarization, P_max and the corresponding wavelength, ${\lambda }_{\max }$. This ${\lambda }_{\max }$ is approximately proportional to average grain size, thereby helping to reveal grain sizes in the intervening medium. We study the average grain sizes in different host galaxies of 4 Type Ia and 10 Type II supernovae through spectropolarimetric observations at multi-wavelengths and compare with the average grain sizes in the diffused interstellar medium of our galaxy. We use archival P_max, ${\lambda }_{\max }$ and width of peak of polarization curve (K) values from the literature. We plot P_max versus ${\lambda }_{\max }$ in color scale that represents K and find that grain sizes of some of the galaxies are smaller, some nearly comparable and some larger than typical grain size (≈5500 Å) of our galaxy. This gives us an insight into the different grain properties especially their sizes in external galaxies compared to our galaxy.